The radial oscillations of neutron stars

Details The radial oscillations of neutron stars The radial oscillations of neutron stars

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apjs...53...93g&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 53, Sept. 1983, p. 93-103. Research supported by the Natural Scie

Physics

26

Equations Of State, Neutron Stars, Radial Distribution, Stellar Oscillations, Vibration Mode, Density Distribution, Frequencies, Matter (Physics), Nuclear Quadrupole Resonance, Pulsars

Scientific paper

The investigation of the influence of the equation of state of matter (in the nuclear density regime) on the dynamical behavior of neutron stars is continued. The properties of the two lowest frequency radial oscillation modes of neutron stars, constructed from 13 equations of state, are presented. It is found that the frequencies of both radial oscillation modes studied here are generally higher than the frequency of the corresponding quadrupole f-mode.

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